1. A Synchronized Two-Dimensional α - Ω Model of the Solar Dynamo.
- Author
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Klevs M, Stefani F, and Jouve L
- Abstract
We consider a conventional α - Ω -dynamo model with meridional circulation that exhibits typical features of the solar dynamo, including a Hale-cycle period of around 20 years and a reasonable shape of the butterfly diagram. With regard to recent ideas of a tidal synchronization of the solar cycle, we complement this model by an additional time-periodic α -term that is localized in the tachocline region. It is shown that amplitudes of some decimeters per second are sufficient for this α -term to become capable of entraining the underlying dynamo. We argue that such amplitudes of α may indeed be realistic, since velocities in the range of m s
-1 are reachable, e.g., for tidally excited magneto-Rossby waves., Supplementary Information: The online version contains supplementary material available at 10.1007/s11207-023-02173-y., Competing Interests: Competing interestsThe authors declare no competing interests., (© The Author(s) 2023.)- Published
- 2023
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